Variations of physical parameters in circumstellar envelopes around carbon-rich Mira variables

Details Variations of physical parameters in circumstellar envelopes around carbon-rich Mira variables Variations of physical parameters in circumstellar envelopes around carbon-rich Mira variables

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..283..239s&link_type=abstract

In: Mass-losing pulsating stars and their circumstellar matter. Workshop, May 13-16, 2002, Sendai, Japan, edited by Y. Nakada, M

Astronomy and Astrophysics

Astrophysics

Circumstellar Matter, Mira Variables, Pulsation

Scientific paper

We have studied variations of physical parameters in the circumstellar envelope of carbon-rich Mira variables at different pulsation phases. After comparing the ISO/SWS spectra of carbon-rich Miras with spectral energy distributions (SEDs) calculated in models, we could find the best fitted parameters for the physical state of the dust envelope at each phase.

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